%0 Conference Paper
%A Kilminster, Ben
%A Aguilar-Arevalo, Alexis
%A Amidei, Dan
%A Bertou, Xavier
%A Butner, Melissa
%A Cancelo, Gustavo
%A Chavarria, Alvaro E.
%A D'Olivo, Juan Carlos
%A Estrada, Juan
%A Fernandez Moroni, Guillermo
%A Izraelevitch, Federico
%A Langisetty, Yashmanth
%A Liao, Junhui
%A Molina, Jorge
%A Privitera, Paolo
%A Salazar, Carolina
%A Sarkis, Youssef
%A Scarpine, Vic
%A Schwarz, Tom
%A Sofo Haro, Miguel
%A Tiffenberg, Javier
%A Trillaud, Frederic
%A Zhou, Jing
%T The DAMIC-100 dark matter detection experiment with CCDs at SNOLAB
%C Hamburg
%I Verlag Deutsches Elektronen-Synchrotron
%M PUBDB-2016-05903
%@ 978-3-935702-59-1
%B DESY-PROC
%P 25-28
%D 2014
%< Kilminster, Ben "The DAMIC-100 dark matter detection experiment with CCDs at SNOLAB " in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014)  / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva
%X The DAMIC (Dark Matter in CCDs) experiment uses the fully depleted silicon of CCDs (Charge Coupled Devices) as a target for galactic dark matter. The ionization energy threshold for detecting nuclear recoils of dark matter reaches down to 50 eV<sub>ee</sub>, resulting in better sensitivity to dark matter with mass below 5 GeV than other direct dark matter detection experiments. Installation of the DAMIC-100 experiment at SNOLAB is ongoing and we present our expected sensitivity, which will extend the reach to low-mass dark matter cross sections within a year of operation.
%B 10th Patras Workshop on Axions, WIMPs and WISPs
%C 29 Jun 2014 - 4 Jul 2014, Geneva (Switzerland)
Y2 29 Jun 2014 - 4 Jul 2014
M2 Geneva, Switzerland
%F PUB:(DE-HGF)8 ; PUB:(DE-HGF)7
%9 Contribution to a conference proceedingsContribution to a book
%R 10.3204/DESY-PROC-2014-03/kilminster_ben
%U https://bib-pubdb1.desy.de/record/315496